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Introduction to Health Physics: Fourth Edition - Ruang Baca FMIPA UB

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HEALTH PHYSICS INSTRUMENTATION 471<br />

Figure 9-30. Diagram of a long<br />

counter, a neutron counter whose<br />

response is approximately uniform from<br />

about 10 keV <strong>to</strong> 5 MeV. (Reproduced<br />

with permission from Hanson AO,<br />

McKibben JL. A neutron detec<strong>to</strong>r having<br />

uniform sensitivity from 10 kev <strong>to</strong> 3<br />

Mev. Phys Rev. 1947; 72(8):673–677.<br />

Copyright c○ 1947 American physical<br />

Society.)<br />

the counter. The counter is enclosed in a thin sheet of cadmium <strong>to</strong> absorb thermal<br />

neutrons in order <strong>to</strong> prevent pulses due <strong>to</strong> deuteron recoils following absorption<br />

of thermal neutrons by the hydrogen. The hydrogenous material may also be a<br />

solid, such as paraffin or polyethylene, incorporated in<strong>to</strong> the wall of the counter.<br />

The fast neutrons “knock out” pro<strong>to</strong>ns from these solids, and the pro<strong>to</strong>ns dissipate<br />

their energy in the counter gas. When used in this way as a source of pro<strong>to</strong>ns, the<br />

hydrogenous substance is called a pro<strong>to</strong>n radia<strong>to</strong>r.<br />

The sensitivity for fast neutrons of a pro<strong>to</strong>n recoil counter is very much less than<br />

the sensitivity of a BF3 counter for thermal neutrons. This is true for two reasons:<br />

The cross section of hydrogen for scattering of fast neutrons is very much less than<br />

the slow-neutron capture cross section of 10 B, and also the energy distribution of the<br />

scattered pro<strong>to</strong>ns includes a large fraction of very low energy pro<strong>to</strong>ns. For neutron<br />

energies up <strong>to</strong> about 10 MeV, the scattering of neutrons is isotropic. This means that<br />

the energy of the scattered pro<strong>to</strong>n may vary from zero <strong>to</strong> the energy of the neutron.<br />

The pulses that result from pro<strong>to</strong>ns <strong>to</strong> which little energy was imparted during the collision<br />

are therefore not counted because of the bias against gamma radiation. Above<br />

this threshold, the energy response of the recoil pro<strong>to</strong>n proportional counter is determined<br />

mainly by the energy dependence of the scattering cross section of hydrogen.<br />

Neutron Dosimetry<br />

The dose equivalent from neutrons depends strongly on the energy of the neutrons,<br />

as shown in Table 9-5. We therefore cannot simply convert neutron flux density<br />

(fluence) in<strong>to</strong> dose equivalent unless we know the energy spectral distribution of<br />

the neutrons. For thermal neutrons, of course, the spectral distribution is known, and<br />

aBF3 counter can be calibrated <strong>to</strong> read directly in millirads per hour. For higher<br />

energy neutrons, neither the moderated BF3 long counter with its “flat” energyindependent<br />

response <strong>to</strong> fast neutrons nor the simple pro<strong>to</strong>n-recoil proportional<br />

counter, whose response <strong>to</strong> fast neutrons depends strongly on the scattering cross<br />

section, is suitable for dosimetry.

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